eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

Open Access

Fig. 18

Top: LS periodogram obtained from the combined light curve of SXP 726 shown below. The dashed red line indicates the 99% confidence level. Bottom: background-subtracted and vignetting-corrected light curve of SXP 726 (binned at twice the pulse period) in the energy band of 0.2–8 keV.

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